[meteorite-list] New MESSENGER Mercury Images

From: Jeff Kuyken <info_at_meteoritecentral.com>
Date: Fri, 2 Oct 2009 20:18:43 +1000
Message-ID: <3D79E729906046FDBDACEFD99CD6C555_at_JeffPC>

Thanks for posting this Ron. The article mentions at "the center of the
bright halo is an irregular depression, which may have formed through
volcanic processes." I'm certainly no expert but the shape appears more like
a double crater. Although admittedly it doesn't look like there is much of a
rim. It will be interesting to see more pics of this region as Messenger
continues its mission.

http://messenger.jhuapl.edu/gallery/sciencePhotos/pics/CN0162744128M_raw.jpg

Cheers,

Jeff


----- Original Message -----
From: "Ron Baalke" <baalke at zagami.jpl.nasa.gov>
To: "Meteorite Mailing List" <meteorite-list at meteoritecentral.com>
Sent: Friday, October 02, 2009 6:07 AM
Subject: [meteorite-list] New MESSENGER Mercury Images



http://messenger.jhuapl.edu

MESSENGER Mission News
October 1, 2009

NEW MESSENGER MERCURY IMAGES

A Bright Spot in the Latest Imaging

Humans have now had three views of the bright area shown near the top center
of this
image
<http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?gallery_id=2&image_id=336>.
The first view was as a mere tiny bright spot seen in telescopic images
of Mercury obtained from Earth by astronomer Ronald Dantowitz. The second
view
<http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?page=3&gallery_id=2&image_id=236>
was obtained by the MESSENGER Narrow Angle Camera during the spacecraft's
second Mercury flyby on October 6, 2008. At that time, the bright feature
was just on the planet's limb (edge) as seen from MESSENGER. Now MESSENGER
has provided a new, even better view. The geometry of MESSENGER's third
Mercury flyby allows us to see the feature and its surroundings in greater
detail, including the smooth plains in the foreground and the rim of a
newly discovered impact basin
<http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?gallery_id=2&image_id=332>
at lower left. Surprisingly, at the center of the bright halo is an
irregular
depression, which may have formed through volcanic processes. Color images
from MESSENGER's Wide Angle Camera reveal that the irregular depression
and bright halo have distinctive color. This area will be of particular
interest for further observation during MESSENGER's orbital operations
starting in 2011.

Evening Shadows

These images
<http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?gallery_id=2&image_id=337>
were taken on approach to Mercury during the spacecraft's second (left)
and third (right) flybys. The image from the second flyby was featured
in an earlier release
<http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?page=1&gallery_id=2&image_id=287>.
The image on the right was taken about 75 minutes before MESSENGER's closest
approach. The two images cover very nearly the same terrain, but for the
right image the Sun's illumination is more nearly grazing (local time
is almost sunset) and the viewing perspective of the spacecraft is more
nearly vertical. The large impact crater bisected with a prominent scarp
or cliff is the same feature in both images. Because of Mercury's rotation
between the two encounters, the position of the crater in the right image
is nearly at the terminator (the division between the dayside and night
side of the planet), and thus the shadows are longer. The near-grazing
illumination emphasizes the topography of the crater floor, including
the relief of the wrinkle ridges on either side of the large scarp. To
the west of the crater, the shadows and viewing angle show that the terrain
is far more rugged than it appeared from the second flyby.

Seeing Double?

This image
<http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?gallery_id=2&image_id=338>
shows a double-ring impact basin, with another large impact crater on
its south-southwestern side. Smaller, more recent impacts formed
comparatively
fresh craters across the entire surface visible in this image. The floor
within the inner or peak ring appears to be smoother than the floor between
the peak ring and the outer rim, possibly the result of lava flows that
partially flooded the basin some time after impact. Double-ring basins
are formed when a large meteoroid strikes the surface of a rocky planet.

Crater Ejecta and Chains of Secondary Impacts

This newly observed flat-floored crater
<http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?gallery_id=2&image_id=339>
was viewed at an oblique angle as MESSENGER approached Mercury for its
third flyby, about two hours from closest approach. This crater is younger
than nearby craters of similar size, indicated by the distinctive halo
of small secondary craters that radiate outward from the central structure.
Many of these secondaries are aligned in chain-like formations and some
show characteristic "herringbone" features pointing back to the crater
of origin. Crater chains are just one of many ejecta types observed on
Mercury. Other ejecta features include distinct continuous ejecta
<http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?image_id=311>
and crater rays
<http://messenger.jhuapl.edu/gallery/sciencePhotos/image.php?image_id=280>,
which are composed of both ejecta and secondaries. Another ejecta feature
of note in this mosaic of two images is a zone of lighter terrain extending
a bit west of north from the crater itself, possibly providing information
about the direction of impact. This unnamed crater is partially superposed
on an older and smaller crater to the south.

Additional information and features from this encounter will be available
online at http://messenger.jhuapl.edu/mer_flyby3.html.
Be sure to check back frequently to see the latest released images and
science results!

________________________________

Highlights from Three Mercury Flybys

Tonight, three MESSENGER team members - Principal Investigator
Sean Solomon, of the Carnegie Institution of Washington, Project Manager
Peter Bedini, of APL, and Co-Investigator Louise Prockter, of APL - will
talk about what we've learned about Mercury from MESSENGER's encounters
with the planet, and release new pictures from the spacecraft's third
flyby of Mercury. The event, to be held at the Kossiakoff Center on the
campus of the Johns Hopkins University Applied Physics Laboratory in Laurel,
Md., will begin at 5 p.m.
________________________________

MESSENGER (MErcury Surface, Space ENvironment, GEochemistry, and Ranging)
is a NASA-sponsored scientific investigation of the planet Mercury and
the first space mission designed to orbit the planet closest to the Sun.
The MESSENGER spacecraft launched on August 3, 2004, and after flybys of
Earth, Venus, and Mercury will start a yearlong study of its target
planet in March 2011. Dr. Sean C. Solomon, of the Carnegie Institution
of Washington, leads the mission as Principal Investigator. The Johns
Hopkins University Applied Physics Laboratory built and operates the
MESSENGER spacecraft and manages this Discovery-class mission for NASA.

________________________________






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Received on Fri 02 Oct 2009 06:18:43 AM PDT